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arXiv · 1205.2001

Non-radial oscillations of neutron stars and the detection of gravitational waves

Cecilia Chirenti·Patrick R. Silveira·Odylio D. Aguiar
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Abstract

We study the non-radial oscillations of relativistic neutron stars, in particular the (fundamental) f-modes, which are believed to be the most relevant for the gravitational wave emission of perturbed isolated stars. The expected frequencies of the f-modes are compared to the sensitivity range of Mario Schenberg, the Brazilian gravitational wave spherical detector.

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Cecilia Chirenti, Patrick R. Silveira, Odylio D. Aguiar. 2012-05-09. Non-radial oscillations of neutron stars and the detection of gravitational waves. https://doi.org/10.1142/s2010194512008185

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